Development of precision Wolter mirrors towards PhoENiX mission for the Sun

T. Sakao, S. Matsuyama, J. Yamada, Takato Inoue, Kentaro Hata, Hiroyuki Yamaguchi, T. Hagiwara, Nami Nakamura, K. Yamauchi, Y. Kohmura, Y. Suematsu, N. Narukage
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Abstract

We present ongoing efforts on the development of precision Wolter mirrors for the Soft X-ray Imaging Spectrometer (SXIS) aboard PhoENiX mission proposed to JAXA for studying mechanism(s) of particle acceleration and its relationship with magnetic reconnection in solar flares. The Wolter mirrors for PhoENiX/SXIS are made by direct polishing of glass-ceramic substrates. So far, we succeeded in fabricating a small size of high precision Wolter surfaces (e.g., PSF core size of ~0.2 arcsec HPD at 8 keV) as well as good indication of extending the mirror area along the cylindrical direction. Recent status of the mirror development will be reported.
为凤凰号太阳任务研制的精密沃尔特反射镜
为了研究太阳耀斑中粒子加速的机理及其与磁重联的关系,我们提出了正在进行的开发用于软x射线成像光谱仪(SXIS)上的菲尼克斯任务的精密Wolter反射镜的努力。用于PhoENiX/SXIS的Wolter反射镜是通过直接抛光玻璃陶瓷基板制成的。到目前为止,我们成功地制造了一个小尺寸的高精度Wolter表面(例如,在8 keV下,PSF核心尺寸为~0.2 arcsec HPD),以及沿圆柱形方向扩展镜面区域的良好迹象。将报告镜像开发的最新情况。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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